Flight Analysis of an Autonomously Navigated Experimental Lander for High Altitude Recovery Jeffrey Chin1, Justin Niehaus2, Debra Goodenow3 NASA Glenn Research Center, Cleveland, OH 44070 Storm Dunker4, David Montague5 Airborne Systems, Santa Ana, CA, 92704 First steps have been taken to qualify a family of parafoil systems capable of increasing the survivability and reusability of high-altitude balloon payloads. The research is motivated by the common risk facing balloon payloads where expensive flight hardware can often land in inaccessible areas that make them difficult or impossible to recover. The Autonomously Navigated Experimental Lander (ANGEL) flight test introduced a commercial Guided Parachute Aerial Delivery System (GPADS) to a previously untested environment at 108,000ft MSL to determine its high-altitude survivability and capabilities. Following release, ANGEL descended under a drogue until approximately 25,000ft, at which point the drogue was jettisoned and the main parachute was deployed, commencing navigation. Multiple data acquisition platforms were used to characterize the return-to-point technology performance and help determine its suitability for returning future scientific payloads ranging from 180 to 10,000lbs to safer and more convenient landing locations. This report describes the test vehicle design, and summarizes the captured sensor data. Various post-flight analyses are used to quantify the system’s performance, gondola load data, and serve as a reference point for subsequent missions. I. Introduction P lanetary science missions often send payloads to near space using balloon gondolas for a fraction of the cost of rockets. These balloon gondolas, however, are usually not reusable after their mission. Expensive flight hardware frequently impacts the ground with high velocities and can sometimes land in inaccessible areas that make them difficult or impossible to recover. A substantial cost and effort savings can be realized by guiding the balloon gondola or its’ experiments to a convenient specified location, away from hazards, after the mission is complete. The flight test is collaboration between engineers at NASA Glenn Research Center (GRC), the Columbia Scientific Balloon Facility (CSBF), and Airborne Systems (AS) as a first step towards qualifying a GPAD system for subsequent scientific missions. The parafoil canopies and Airborne Guidance Unit (AGU) have an expansive flight history for commercial and military missions, typically Parafoil deployed from around 25,000ft via static-line cargo plane drops. GPADS of this scale have never been tested, and scientifically documented, from altitudes of 108,000ft, where the atmosphere is significantly colder and less dense. This flight seeks to characterize the performance of AGU a GPAD system under these harsher environmental conditions and rapid descent speeds. The on-board avionics will monitor the condition of both the navigation system Figure 1. GPADS traditionally deployed from and the payload it carries. aircraft. 1 Aerospace Engineer, Propulsion Systems Analysis Branch, Mail Stop 5-11, AIAA Member 2 Aerospace Engineer, Combustion Physics and Reacting Processes Branch, Mail Stop 77-5, AIAA Member 3 Electrical Systems Engineer, Diagnostics and Electromagnetics Branch, Mail Stop 86-5 4 Parachute Systems Engineer, Airborne Systems, CA, US, AIAA Member 5 Senior Software Engineer, Airborne Systems, NJ, US 1 American Institute of Aeronautics and Astronautics The ANGEL system consists of the drogue, parafoil, AGU, and the Balloon Flight System payload (BFS) subsystems, where the first three form the GPAD system. The individual components and systems overview, as packed, are illustrated in Figure 2. This document describes the post- flight data analysis of the information gathered by the ANGEL avionics platform. This data is used to validate engineering analyses, document lessons learned, and act as reference data for future flights where GPAD systems could provide appreciable benefits. The stored data is used to verify thermal and structural models, as well as validate electrical power system and telemetry performance. The information also serves to measure the gondola’s descent stability and characterize the parafoil performance. The on-board data acquisition platform Figure 2. ANGEL system overview. recorded environmental conditions, measuring the avionics performance and verifying expected impact forces. II. Vehicle and Mission Description Figure 3. Balloon launch. 2 American Institute of Aeronautics and Astronautics The ANGEL system was launched as a piggyback payload on a CSBF Mission of Opportunity on September 4th, 2015 from Fort Sumner, New Mexico. The 6,000lb max gross-weight host vehicle, nicknamed “Thunderbird”, was lifted by a 29 million cubic foot Helium balloon envelope pictured in Figure 3. Figure 4 shows Thunderbird in white with the ANGEL system mounted front and center. The Airborne System drogue, parafoil, and AGU are the yellow components, sitting on top of the Balloon Flight System (BFS) painted orange. The BFS gondola, designed and built at NASA Glenn Research Center, is composed of a beveled rectangular aluminum skeleton reaching a total system weight of 230lbs including the AGU and canopies. During integration, the drogue, parafoil, and AGU are stacked vertically on top of a honeycomb spacer and connected via four tie-down D-rings. The BFS is attached to the Thunderbird gondola by a single eyebolt on the top surface and restricted from motion after release using a guide rail on the side of the gondola seen in Figure 5. An interference pin mounted to the gondola engages the BFS eyebolt. In order to release ANGEL, a linear actuator pulls the interference pin, disengaging the eyebolt, see Figure 6, allowing the ANGEL system to fall from the host vehicle after reaching its floating altitude. After release of the BFS, a four-roller guide on the side of the BFS, shown in red in Figure 5, travels along the rail on the gondola, minimizing pitch, roll, or yaw motion, and improving the likelihood of a straight Figure 4. Thunderbird Gondola. trajectory for ANGEL during release. The drogue static line is fastened through a hole in the top of the separation device housing. During release, the drogue static line is pulled taught and the drogue bridle, drogue, and attenuation stitching are extracted. An attenuation strip applies a near constant force to the apex of the drogue for the first approximately 70 ft of descent. This prevents the drogue from recoiling into the BFS after release and allows the system to build airspeed. Approximately four seconds of freefall was predicted as necessary to build sufficient dynamic pressure to inflate the drogue. ANGEL then intended to descend under drogue for approximately 400 seconds, keeping the payload stable and below Mach 1 until it reaches a GPS trigger altitude of 6,250m (20,505ft) above the programmed IP elevation. For the area being tested, the trigger altitude is about 7,620m (25,000ft) MSL. At this point the AGU commands the release of the drogue using a dedicated motor, and the drogue is jettisoned, while simultaneously deploying the main parafoil. The drogue and deployment bag separate from the main canopy by design. The AGU then commences GPS navigation using standard GPADS flight software. The parafoil is controlled using motors contained within the AGU. In the event of a GPS lock loss, a timer backup was present to trigger the drogue release and main parachute deployment. All active control sensors were located within the Airborne Guidance Unit, with all redundant data acquisition systems contained within the gondola. Redundant GPS and multiple cameras were placed on the corners of the top plate, with streaming 2-way telemetry antennae located on the bottom face. Live two-way telemetry and video feed were used to monitor and log the system status and trajectory. Data was gathered starting in the pre-launch segment, through ascent and descent and logged to multiple on-board storage devices and ground stations. 3 American Institute of Aeronautics and Astronautics Figure 5. (Left) Front side of the BFS with separation carriage in red. (Right) Actual system being mounted to the host vehicle guide rail. Figure 6. The payload is secured vertically from a single 1" diameter steel pin. 4 American Institute of Aeronautics and Astronautics III. GPADS Objectives Concerning the advancement of GPADS technology to space recovery applications, the ANGEL test has provided the opportunity to test this GPAD system at conditions not previously possible. Specifically, the challenges to surmount include: Operating electro-mechanical systems at combined low densities and low temperatures Textile tolerance to radiation exposure Safely and reliably releasing the payload and the subsequent inflation of the drogue Remaining under Mach 1 and transonic regimes during droguefall Using GPS sensors at or beyond their altitude limits Mission Planning for large offset balloon flights A. Thermal Management Due to the combination of low temperature and low density, design attention was given to the battery packs in the AGU. Too low of an operating temperature will quickly drain and potentially damage the Li-ion batteries. A common minimum safe operating temperature is -20C. The GPS receiver had a minimum operating temperature of - 40C. Accordingly, the airborne guidance unit included a thermostatically controlled battery heating system. This configuration was designed and environmentally tested to function over the ascent and descent to/from 100,000-ft MSL. The warming function would turn on when the internal temperature dropped below a pre-selected temperature. The GPS receiver chip was not directly thermally controlled, but confidence was provided in the form of successful environmental tests. It was thus a critical objective that the batteries health to be maintained throughout the flight envelope. From previous flights at lower altitudes, where the thermal management system was first tested, overheating due to reduced thermal capacity of air was not expected to be an issue. The AGU draws relatively little power during ascent, and during descent, wind chill plays a dominant role. B. Textile Exposure Textiles react strongly to UV light exposure. Normal exposure rates at earths surface can require days to observe degredation to material properties. However, at higher altitudes, with less filtering performed by the atmosphere, increased exposure to light and radiation sources were expected to accelerate the degredation process. As a result, lighter colors were selected for textile components since they absorb less light, material strengths were intentially overbuilt, and a minimum of structural elements were left uncovered by deployiment bags. It was thus anticipated that significant tolerance to material degredation was present in the design of the system. However, longer duration missions will likely require light and radiation barrier protection until the time when the system would be used. A GPADS objective was therefore to demonstrate that the materials selected and methods of textile protection were adequate for short duration balloon missions. Figure 7. ANGEL Packed and Rigged 5 American Institute of Aeronautics and Astronautics C. Safe Release Of critical importance to the ANGEL flight was to have a safe and controlled release from the host vehicle. Fouling a release could result in a loss of all mission objectives. On release of the ANGEL mass, in addition to some balloon dynamics, the gondola rotates so that the new CG (less the ANGEL system) is directly beneath the balloon tether. Initially conceived separation mechanisms posed a potential risk for the lowest portion of the gondola to possibly re-contact the BFS or parachutes by rotating into them as they fell by. With this ‘kick’, the ANGEL system could theoretically rotate as a mass in motion for 4 or more seconds until a suitable stabilizing force was available from the drogue, by which time, the drogue bridle could be wrapped up and tangled on the payload. Furthermore, due to the lack of real estate on the top face of the BFS and the requirement to keep the parachutes clear of obstruction, all vertical forces were concentrated through single cantilevered eyebolt and pin. A dual pin system (one in each back corner) was considered, but ultimately deemed more likely to fail or induce rotation upon release. The final release design implemented the single pin and rail system, previously discussed, minimizing any rotation induced by the abrupt release. Parachute deployments in low density atmosphere are known to have unique inflation characteristics. Particularly important is the need to manage rebound after elongation of the flexible elastic textile structure (risers, lines, and gores) due to conservation of momentum between payload and the drogue itself. There are documented cases where the parachute has rebounded to be below the payload (i.e. closer to earth than the payload), which is especially dangerous as it could tangle on the payload itself and compromise the entire flight. The design of deployment was therefore important. As a preventative measure, a load attenuation strip was added between the drogue and the drogue deployment bag. This attenuation strip would peel for about 85 ft of payload descent. A longer distance was desired, but not permitted at the time. It would be desirable to maintain attenuation until sufficient dynamic pressure could be achieved to inflate the drogue. A GPADS objective for the ANGEL drop was to prove the pin and rail release systems by having a clean release from the host gondola, with no rotation motion or re-contact with the gondola after release. Further, it was also an objective that the drogue remain above the payload at all times. D. Descent Speed Control Fundamentally, a decision was made early to avoid Mach 1 and transonic speeds to prevent sonic boom shock wave, forebody vibrations, changes to drogue performance, and other challenges. At the time of architecture selection, the planned release was to be from 130,000ft. A 9.85 ft D ribbon parachute was selected as the preferred drogue which would O ensure velocity < Mach 0.75 if dropped from 130,000ft. The release altitude was later reduced to 105,000ft, which only provides more margin. This drogue is a mature qualified design which has a known performance at lower altitudes. A secondary objective of the ANGEL drop was to characterize the drogue’s opening, stability, and descent rate performance at these yet-tested higher altitudes. To understand the droguefall performance with an ANGEL representative payload configuration, a C characterisation test was D performed. This information was important to ensure both Mach limits were maintained as well as calculating the correct droguefall time for the backup timer functionality. Figure 8. Drogue CD Characterization Test E. GPS in Adverse Conditions Because the planned altitude of the test, there was uncertaintly how the U-blox GPS module would perform. As a result of the concern wether the AGU would lose GPS lock at higher altitudes and regain it, or not, during high- speed descent, a backup timer was added as an either / or condition with the 25,000ft MSL GPS altitude trigger. An 6 American Institute of Aeronautics and Astronautics objective of the test was then to prove out the GPS functionality and the programming logic for deployment of the main parachute. GPS reception was also a concern given the presence of multiple other communication systems and the large metal body of the vehicle itself. During integration it was discovered that an external antenna and filter was necessary to maintain GPS lock when exposed to CSBF communication signals. F. Mission Planning Mission planning is routine for existing commercial applications of GPADS. However, special efforts were required to assist the ANGEL mission. Due to the nature of balloon flight, where the system blows with the wind, it is never precisely certain what the ascent trajectory will look like, or where the release location will be. Consequently, numerous hazard restrictions were levied onto ANGEL. Hazard avoidance included the following restrictions, shown in Figure 14: 8 nm diameter No-fly zones near population centers – entire failure footprint (red circles) 4 nm keep out zones from roads, highways, interstates, and high tension power lines – entire failure footprint 1 nm diameter keep out zones from dwellings (inhabited or uninhabited) – ballistic failure footprint (purple circles) As a result of the uncertain ascent path, there was the expectation that release would be decided on-the-fly when the ballistic footprint was acceptable. Therefore, the decision to release places a higher priority on safety than accuracy of landing. Prior to the first launch window, suitable impact points (IP’s) were sought and surveyed, based on anticipated ascent trajectory. This involved a day or two of scouting safe, accessible land with landowner consent. However for the actual launch day there was not sufficient time based on changed wind conditions and personnel availablility to scout for IPs. The GPADS objective for mission planning was for the ANGEL to land within 150 meters of a pre-selected landing point based on the predicted ascent trajectory and release point, while successfully avoiding the hazards identified. 7 American Institute of Aeronautics and Astronautics IV. Passive BFS Data Acquisition System Balloon Flight System Components: 1. NASA Gondola 2. NASA Impact Sensors 3. NASA Battery 4. NASA PMAD 5. NASA Avionics 6. NASA Radio 7. NASA GPS 8. Airborne Systems Antenna 9. NASA Antennae 10. Thermal Foam 11. Go-Pro Camera Systems 12. Eye Bolt 13. Tie-Down Rings 14. Subsystem Shelf 15. Separation Carriage Figure 9. (Above) CAD model showing the internal arrangement of BFS sensors. Figure 10. (Left) Isometric view, with insulation hidden. Arrays of sensors were contained within the aluminum BFS frame to record the flight from the perspective of the test payload. This passive data acquisition system was used to measure the GPAD performance and quantify the flight loads. The platform consisted of a power source, radio, sensors, flight computer, insulation, and ballast. A three-cell battery pack each comprised of 5 series connected SAFT B0562 Lithium Sulfur Dioxide batteries were enclosed within a passive thermally controlled foam shell. Power was distributed from the battery using a custom power management and distribution (PMAD) board connected to the data acquisition units, and radio transmitter. The data acquisition units were comprised of the following sensors types: 1) GPS- Measure position, altitude, velocity, heading and time 2) Accelerometers- 3D accelerations, vibration loads and orientation 3) Gyros- Orientation and angular velocity 4) Magnetometers- Aid in calculating heading and IMU sensor fusion 5) Thermocouples- Monitor temperature of electronics 6) Cameras- Visual feedback 7) Current/Voltage Monitoring- Battery performance Each of these sensors was redundantly measured from multiple locations and multiple power sources. All BFS sensors were independent from the sensors inside the AGU that were used to actively navigate the payload on descent. This system also periodically broadcasted and received telemetry data from a ground station located along the projected mission path. The two secondary data acquisition (DAQ) systems passively monitored gondola conditions from inside the blue structure in Figure . These sensors provided redundancy, along with a secondary perspective on the flight loads while the AGU was suspended above the gondola during its final glide segment. One of the internal DAQ systems also continuously streamed data to ground stations to help monitor the payload status. This secondary radio system helped ensure maximum data recovery, even if the payload were to be destroyed on impact. 8 American Institute of Aeronautics and Astronautics V. Results A. Day of Flight Conditions A regional weather forecast was used to plan for acceptability of landing locations. The temperature, wind speed, and wind heading conditions predicted for the flight are shown in Figure 11 below. The inherent canopy forward airspeed of the parafoil, based on the suspended weight, is also displayed to demonstrate that the forecast wind is about half of the speed of the system for the portion of altitudes using the parafoil. Figure 11. CSBF Forecast for the Area. 9 American Institute of Aeronautics and Astronautics B. Launch After a two-hour prelaunch inflation period, the host vehicle was launched at 6:50am. Given the size of the balloon and payload, pendulum effect during release was eliminated by driving the payload until it was directly beneath the balloon at release. This ground vehicle, nicknamed “Big Bill”, can be seen in Figure 12 as the balloon began to ascend. Figure 12. View from just after Launch from Thunderbird. During this release, the payload experienced a 3 g vertical acceleration and 3 Hz dampening vibration as shown in Figure . At this point the internal temperature was approximately 90°F with a max rotational speeds of 0.26 rad/s occurring. Figure 13. Launch Vibrations. 10 American Institute of Aeronautics and Astronautics